| 书目名称 | Properties and Interactions of Interplanetary Dust |
| 副标题 | Proceedings of the 8 |
| 编辑 | R. H. Giese,P. Lamy |
| 视频video | http://file.papertrans.cn/762/761315/761315.mp4 |
| 丛书名称 | Astrophysics and Space Science Library |
| 图书封面 |  |
| 描述 | Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth‘s environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort |
| 出版日期 | Conference proceedings 1985 |
| 关键词 | Corona; Heliosphere; Planet; Solar; Solar System; Solar wind; Sun |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-94-009-5464-9 |
| isbn_softcover | 978-94-010-8912-8 |
| isbn_ebook | 978-94-009-5464-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 |
| issn_series | 0067-0057 |
| copyright | Springer Science+Business Media Dordrecht 1985 |
|Archiver|手机版|小黑屋|
派博传思国际
( 京公网安备110108008328)
GMT+8, 2025-7-23 00:46
发表于 2025-3-21 19:15:49
